Zobrazeno 1 - 10
of 85
pro vyhledávání: '"S P Fox"'
Autor:
S. N. Fox, L. J. McMeekin, C. H. Savage, K. L. Joyce, S. M. Boas, M. S. Simmons, C. B. Farmer, J. Ryan, L. Pereboeva, K. Becker, J. Auwerx, S. Sudarshan, J. Ma, A. Lee, R. C. Roberts, D. K. Crossman, A. Kralli, R. M. Cowell
Publikováno v:
npj Parkinson's Disease, Vol 8, Iss 1, Pp 1-19 (2022)
Abstract Many studies implicate mitochondrial dysfunction as a key contributor to cell loss in Parkinson disease (PD). Previous analyses of dopaminergic (DAergic) neurons from patients with Lewy-body pathology revealed a deficiency in nuclear-encoded
Externí odkaz:
https://doaj.org/article/ea2bd0f17cd2417ea87f86dbe8b0be2d
Publikováno v:
Virtual and Physical Prototyping, Vol 14, Iss 2, Pp 148-159 (2019)
This paper characterises the flexural properties of relatively slender structural members (beams) manufactured using a FDM-based 3D printer. The primary goal is to assess the influence of infill properties on flexural rigidity through a parametric in
Externí odkaz:
https://doaj.org/article/22ef36d706eb4adab6ba8903fab10461
Publikováno v:
Developmental Cognitive Neuroscience, Vol 35, Iss , Pp 28-35 (2019)
In adults, affective touch leads to widespread activation of cortical areas including posterior Superior Temporal Sulcus (pSTS) and Inferior Frontal Gyrus (IFG). Using functional Near Infrared Spectroscopy (fNIRS), we asked whether similar areas are
Externí odkaz:
https://doaj.org/article/42ba4b1ae6f54a68a70c170c22882c75
Autor:
S. Lloyd-Fox, K. Begus, D. Halliday, L. Pirazzoli, A. Blasi, M. Papademetriou, M.K. Darboe, A.M. Prentice, M.H. Johnson, S.E. Moore, C.E. Elwell
Publikováno v:
Developmental Cognitive Neuroscience, Vol 25, Iss , Pp 92-104 (2017)
Brain and nervous system development in human infants during the first 1000 days (conception to two years of age) is critical, and compromised development during this time (such as from under nutrition or poverty) can have life-long effects on physic
Externí odkaz:
https://doaj.org/article/3834d5ef85a140bb91187b1921dfce56
Autor:
I. Matea, A. Gottardo, I. Sivacek, Mahmoud Mahgoub, M. Assié, S. Gillespie, L. Olivier, F. Hammache, M. Degerlier, V. Alcindor, I. Stefan, C. Delafosse, Didier Beaumel, A. Georgiadou, Jérôme Guillot, R. Garg, Marin Chabot, J. Riley, T. Faestermann, Alison Laird, L. Perrot, Valdir Guimaraes, F. Flavigny, Ralf Hertenberger, J. Kiener, P. Adsley, A. Lefebvre-Schuhl, N. de Sereville, Vincent Tatischeff, H.-F. Wirth, Arnd Meyer, S. P. Fox
Publikováno v:
Physical Review C. 103
Spatially-correlated overabundances of $^{15}$N and $^{18}$O observed in some low-density graphite meteoritic grains have been connected to nucleosynthesis taking place in the helium-burning shell during core-collapse supernovae. Two of the reactions
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::105116125c9e5b2cda32407243b99e31
https://doi.org/10.1103/physrevc.103.035804
https://doi.org/10.1103/physrevc.103.035804
Autor:
Giuseppe Verde, Mark A. Williams, Alison Laird, M. Assié, R. Garg, S. Gillespie, Vincent Tatischeff, Anuj Parikh, A. Lefebvre-Schuhl, J. Riley, N. de Sereville, A. Remadi, S. Franchoo, N. J. Hubbard, C. Hamadache, I. Stefan, J. Kiener, F. Hammache, L. Perrot, B. Bastin, F. de Oliveira Santos, S. P. Fox, F. Boulay, Daisuke Suzuki, Valdir Guimaraes, P. Adsley, A. Coc
Publikováno v:
Physical Review C. 103
Classical novae result from thermonuclear explosions producing several $\gamma$-ray emitters which are prime targets for satellites observing in the MeV range. The early 511 keV gamma-ray emission depends critically on the $^{18}$F(p,$\alpha$)$^{15}$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::24dead5e4a3385b0c2277589f51e07d4
https://doi.org/10.1103/physrevc.103.015807
https://doi.org/10.1103/physrevc.103.015807
Autor:
S. P. Fox, Alison Laird, Marco Pignatari, N. J. Hubbard, Anuj Parikh, A. M. Howard, M. Munch, Oliver S. Kirsebom, C. Aa. Diget, J. R. Tomlinson, H. O. U. Fynbo
Publikováno v:
Hubbard, N J, Diget, C A, Fox, S P, Fynbo, H O U, Howard, A M, Kirsebom, O S, Laird, A M, Munch, M, Parikh, A, Pignatari, M & Tomlinson, J R 2021, ' New Experimental 23 Na(α, p) 26 Mg Reaction Rate for Massive Star and Type Ia Supernova Models ', The Astrophysical Journal, vol. 912, no. 1, 59 . https://doi.org/10.3847/1538-4357/abee91
The $^{23}$Na($\alpha,p$)$^{26}$Mg reaction has been identified as having a significant impact on the nucleosynthesis of several nuclei between Ne and Ti in type-Ia supernovae, and of $^{23}$Na and $^{26}$Al in massive stars. The reaction has been su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::867a7160c14a6f9a556e34c82f8d7b5b
https://mediatum.ub.tum.de/doc/1653669/document.pdf
https://mediatum.ub.tum.de/doc/1653669/document.pdf
Autor:
L. Buchmann, B. R. Fulton, N. Galinski, Jennifer Fallis, A. Chen, Jun Chen, B. Davids, C. Akers, S. Sjue, Uwe Greife, D. J. Mountford, S. Reeve, M. Williams, D. A. Hutcheon, C. Davis, L. Erikson, Marco Pignatari, Götz Ruprecht, Raphael Hirschi, Kelly Chipps, D. Howell, L. Martin, Chris Ruiz, D.F. Ottewell, M. Taggart, Urs Frischknecht, Laurelle Veloce, J. R. Brown, C. Aa. Diget, U. Hager, Arthur Choplin, Alison Laird, John D'Auria, S. P. Fox, M. A. Bentley, A. St. J. Murphy
Publikováno v:
Taggart, M P, Akers, C, Laird, A M, Hager, U, Ruiz, C, Hutcheon, D A, Bentley, M A, Brown, J R, Buchmann, L, Chen, A A, Chen, J, Chipps, K A, Choplin, A, D'Auria, J M, Davids, B, Davis, C, Diget, C A, Erikson, L, Fallis, J, Fox, S P, Frischknecht, U, Fulton, B R, Galinski, N, Greife, U, Hirschi, R, Howell, D, Martin, L, Mountford, D, Murphy, A S J, Ottewell, D, Pignatari, M, Reeve, S, Ruprecht, G, Sjue, S, Veloce, L & Williams, M 2019, ' A direct measurement of the 17O(a,g)21Ne reaction in inverse kinematics and its impact on heavy element production ', Physics Letters B, vol. 798 . https://doi.org/10.1016/j.physletb.2019.134894, https://doi.org/10.1016/j.physletb.2019.134894
Physics Letters B, Vol 798, Iss, Pp-(2019)
Physics Letters B, Vol 798, Iss, Pp-(2019)
During the slow neutron capture process in massive stars, reactions on light elements can both produce and absorb neutrons thereby influencing the final heavy element abundances. At low metallicities, the high neutron capture rate of 16-O can inhibit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1c47f576749b9c6a3ad52b1f28477d4
http://arxiv.org/abs/1910.00870
http://arxiv.org/abs/1910.00870
Autor:
A. Georgiadou, A. Gottardo, Alison Laird, N. Oulebsir, Á. M. Sánchez Benítez, F. Flavigny, J. Kiener, A. Coc, F. de Oliveira, J. Riley, D. Beaumel, M. MacCormick, L. Olivier, J. Guillot, L. Grassi, I. Matea, N. Hubbard, Giuseppe D’Agata, C. Delafosse, K. Béroff, Valdir Guimaraes, L. Perrot, S. P. Fox, P. Adsley, N. de Séréville, C. Portail, F. Hammache, A. Meyer, Anuj Parikh, Alessandro Luiz Lara, V. Tatischeff, M. Assié, T. Id Barkach, Marlete Assunção, I. Stefan, B. Bastin
Publikováno v:
Springer Proc.Phys.
15th International Symposium on Nuclei in the Cosmos
15th International Symposium on Nuclei in the Cosmos, Jun 2018, Assergi, Italy. pp.195-200, ⟨10.1007/978-3-030-13876-9_32⟩
Springer Proceedings in Physics ISBN: 9783030138752
15th International Symposium on Nuclei in the Cosmos
15th International Symposium on Nuclei in the Cosmos, Jun 2018, Assergi, Italy. pp.195-200, ⟨10.1007/978-3-030-13876-9_32⟩
Springer Proceedings in Physics ISBN: 9783030138752
International audience; The$^{30}$ P(p, $\gamma $ )$^{31}$ S reaction is one of the few remaining reactions whose rate uncertainty has a strong impact on classical novae model predictions. To reduce the nuclear uncertainties associated to this reacti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3168b7f70a0cba6235c0e8ddcdc2815
https://hal.archives-ouvertes.fr/hal-02317359
https://hal.archives-ouvertes.fr/hal-02317359
Autor:
P. Adsley, Anne Meyer, H.-F. Wirth, Ralf Hertenberger, J. W. Brümmer, R. Neveling, Thomas Faestermann, D. Seiler, Fairouz Hammache, N. de Séréville, S. P. Fox
Publikováno v:
Physical Review C. 97
Background: The Ne-22(alpha, n)Mg-25 reaction is an important source of neutrons for the s-process. Direct measurement of this reaction and the competing Ne-22(alpha,gamma)Mg-26 reaction are challenging due to the gaseous nature of both reactants, th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bbe34eb0e4a2458a5938966495cc4e42
https://doi.org/10.1103/physrevc.97.045807
https://doi.org/10.1103/physrevc.97.045807